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Cited article:

Gaia uncovers difference in B and Be star binarity at small scales: evidence for mass transfer causing the Be phenomenon

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Monthly Notices of the Royal Astronomical Society 527 (2) 3076 (2023)
https://doi.org/10.1093/mnras/stad3105

Velocity monitoring of γ Cas stars reveals their binarity status

Yaël Nazé, Gregor Rauw, Stefan Czesla, Myron A Smith and Jan Robrade
Monthly Notices of the Royal Astronomical Society 510 (2) 2286 (2022)
https://doi.org/10.1093/mnras/stab3378

γ Cas stars: Normal Be stars with discs impacted by the wind of a helium-star companion?

N. Langer, D. Baade, J. Bodensteiner, et al.
Astronomy & Astrophysics 633 A40 (2020)
https://doi.org/10.1051/0004-6361/201936736

Let there be more variability in two γ Cas stars

Yaël Nazé, Andrzej Pigulski, Gregor Rauw and Myron A Smith
Monthly Notices of the Royal Astronomical Society 494 (1) 958 (2020)
https://doi.org/10.1093/mnras/staa617

Suzaku and NuSTAR X-ray spectroscopy of γ Cassiopeiae and HD 110432

Masahiro Tsujimoto, Kumiko Morihana, Takayuki Hayashi and Takao Kitaguchi
Publications of the Astronomical Society of Japan 70 (6) (2018)
https://doi.org/10.1093/pasj/psy111

THE ORIGIN OF THE PUZZLING HARD X-RAY EMISSION OFγCASSIOPEIAE

Christian Motch, Raimundo Lopes de Oliveira and Myron A. Smith
The Astrophysical Journal 806 (2) 177 (2015)
https://doi.org/10.1088/0004-637X/806/2/177

STATISTICAL ANALYSIS OF INTERFEROMETRIC MEASUREMENTS OF AXIS RATIOS FOR CLASSICAL Be STARS

R. P. Cyr, C. E. Jones and C. Tycner
The Astrophysical Journal 799 (1) 33 (2015)
https://doi.org/10.1088/0004-637X/799/1/33